词条 | Mons (planetary nomenclature) |
释义 |
The term tholus ("dome") is used for names of smaller (especially domical) uplands, and the term colles ("hills") in names of groups of still smaller knobs. Peculiar round mountains found on Venus get names with the term farrum.[3] Nature of montesThe term mons, like other terms of planetary nomenclature, describes only the external view of the feature, but not its origin or geological structure. It is used for mountains of any origin, and objects in this class are very diverse. Usually they are results of tectonic, impact or volcanic processes. Examples of such mountains are the Maxwell Montes on Venus,[4] the Montes Apenninus on the Moon and Olympus Mons on Mars,[6] respectively. More unusual origins are also possible. For example, the Geryon Montes of Mars are an erosional remnant of a former plateau within Ius Chasma, part of the Valles Marineris canyon system. During impact events, mountains can appear not only on the border of the resulting crater, but also in its center. Classical central peaks generally are not named, although some peaks within craters are named: for example, Aeolis Mons within Gale crater on Mars or the Scheria Montes within Odysseus crater on Tethys. Names of montesThe term mons was firstly used for extraterrestrial mountains by Michael van Langren in 1645.[7] He assigned names to some mountains on the Moon,[2] but none of these names remain in use.[9] Two years later Johannes Hevelius proposed[10] the first names of extraterrestrial mountains still used. The lunar Alps and Apennines still bear names given by Hevelius, and five of his other mountain names nowadays refer to other features (in some cases his "mountains" later turned out to be bright rays from craters).[11] The International Astronomical Union approved the first names of extraterrestrial mountains (together with many other traditional lunar names) in 1935, although without a generic Latin term, which was restored in 1961.[7] As of May 2015, 262 extraterrestrial mountains and mountain systems have official names: 117 on Venus, 50 on Mars, 48 on the Moon, 23 on Io, 13 on Titan, 9 on Iapetus, 1 on Mercury and 1 on Tethys.[2] They are named differently on different celestial bodies:[2][15]
See also
References1. ^{{cite book | author=Fred W. Price | title=The Moon observer's handbook | publisher=Cambridge University Press | location=London | year=1988 | isbn= 978-0-521-33500-3}} [3][4][5][6][7][8][9][10][11]2. ^Map of the Moon by Michael van Langren (1645) 3. ^1 {{cite web |url = http://planetarynames.wr.usgs.gov/Page/Categories |title = Categories for Naming Features on Planets and Satellites |publisher = International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) |work = Gazetteer of Planetary Nomenclature |accessdate = 2015-05-05 |archiveurl = https://web.archive.org/web/20140708063522/http://planetarynames.wr.usgs.gov/Page/Categories |archivedate = 2014-07-08 |deadurl = no}} 4. ^1 2 3 {{cite web |url = http://planetarynames.wr.usgs.gov |title = Gazetteer of Planetary Nomenclature |publisher = International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) |accessdate = 2015-05-05}} 5. ^1 {{cite web |url = http://planetarynames.wr.usgs.gov/DescriptorTerms |title = Descriptor Terms (Feature Types) |work = Gazetteer of Planetary Nomenclature |publisher = International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) |accessdate = 2015-05-05 |archiveurl = https://www.webcitation.org/6QX6KDIQk?url=http://planetarynames.wr.usgs.gov/DescriptorTerms |archivedate = 2014-06-23 |deadurl = no |df = }} 6. ^1 2 {{cite book |title =Encyclopedia of Planetary Landforms |pages=1–2 |editor1=H. Hargitai |editor2=Á. Kereszturi |chapter =Mons, Montes |author =Hargitai H. |publisher =Springer New York |date =2014 |isbn =978-1-4614-9213-9 |doi =10.1007/978-1-4614-9213-9_240-1 |url =https://link.springer.com/book/10.1007/978-1-4614-9213-9 |chapterurl =https://link.springer.com/referenceworkentry/10.1007/978-1-4614-9213-9_240-1}} 7. ^1 {{cite book |author =Hevelius J. |title =Selenographia sive Lunae descriptio |place =Gedani |publisher=Hünefeld |date =1647 |pages =226–235 |doi =10.3931/e-rara-238 |url =http://www.e-rara.ch/zut/content/pageview/160524}} (list of names — on p.228-235) 8. ^1 {{cite journal|author1=Keep M. |author2=Hansen V. L. |title=Structural history of Maxwell Montes, Venus: Implications for Venusian mountain belt formation |journal=Journal of Geophysical Research |year=1994 |volume=99 |issue=E12 |pages=26015–26028 |url=http://www.d.umn.edu/dees/research/planetaryLab/documents/KeepHansenJGR94.pdf |doi=10.1029/94JE02636 |bibcode=1994JGR....9926015K |deadurl=unfit |archiveurl=https://web.archive.org/web/20150328024728/http://www.d.umn.edu/dees/research/planetaryLab/documents/KeepHansenJGR94.pdf |archivedate=March 28, 2015 }} 9. ^1 {{cite journal |author =Plescia J. B. |title =Morphometric properties of Martian volcanoes |journal=Journal of Geophysical Research |year =2004 |volume =109 |issue =E3 |pages =E03003 |bibcode=2004JGRE..109.3003P |doi =10.1029/2002JE002031}} 10. ^1 {{cite book |title =Mapping and Naming the Moon: A History of Lunar Cartography and Nomenclature |author =Whitaker E. A. |publisher =Cambridge University Press |date =2003 |isbn =9780521544146 |url =https://books.google.com/books?id=aV1i27jDYL8C&pg=PA209&dq=mons%20montes |pages =50–57, 201–209 |bibcode =2003mnm..book.....W}} 11. ^1 {{cite book |title =Mapping and Naming the Moon: A History of Lunar Cartography and Nomenclature |author =Whitaker E. A. |publisher =Cambridge University Press |date =2003 |isbn =9780521544146 |url =https://books.google.com/books?id=aV1i27jDYL8C&pg=PA45&dq=mons%20montes |pages =45–46, 195–200 |bibcode =2003mnm..book.....W}} }} Links
2 : Surface features of bodies of the Solar System|Extraterrestrial mountains |
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